Detection of CH+, CH and H2 Molecules in the Young Planetary Nebula IC 4997-Reference-Cited by-同舟云学术

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Detection of CH+, CH and H2 Molecules in the Young Planetary Nebula IC 4997

Published:2020-06-09 Issue:1013 Volume:132 Page:074201
ISSN:0004-6280
Container-title:Publications of the Astronomical Society of the Pacific
language:
Short-container-title:PASP

Author:

Rao N. Kameswara,Lambert David L.,Reddy Arumalla B. S.,García-Hernández D. A.,Manchado Arturo,Díaz-Luis J. J.

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.1088/1538-3873/ab9097/pdf

Reference50 articles.

1. H2 emission in the low-ionization structures of the planetary nebulae NGC 7009 and NGC 6543

2. Changes in the Planetary Nebula IC 4997

3. Detection of atomic hydrogen in the young planetary nebula IC 4997

4. Spatially Resolved Molecular Hydrogen Emission in the Inner 200 AU Environments of Classical T Tauri Stars

Cited by 4 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. FAST Search for Circumstellar Atomic Hydrogen. I. The Young Planetary Nebula IC 4997;The Astrophysical Journal;2022-06-28

2. An episodically variable stellar wind in the planetary nebula IC 4997;Astronomy & Astrophysics;2022-01

3. Analysis of measured high-resolution doublet rovibronic spectra and related line lists of ¹²CH and ¹⁶OH;Physical Chemistry Chemical Physics;2022

4. Potential UV standards for UVIT filter system;Journal of Astrophysics and Astronomy;2021-07-30

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